DRC and PM-cleaned CMDs of Terzan 5 obtained through the photometric reduction and the differential reddening map described in this work. The left-hand panel displays all the member stars measured in the FOV, while the right-hand panel shows the subsample of stars satisfying our quality cuts, specifically a radial distance of r ≥ 15″ from the center and good values of χ and asharpness (i.e., within 3σ of their distributions; see Fig. 3).